Routine Space Environment Product (Daily)
Issued by NWS

Home |  Current Version |  Previous Version |  Text Only |  Print | Product List |  Glossary On
Versions: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15
855
FXXX12 KWNP 301231
DAYDIS

:Product: Forecast Discussion
:Issued: 2024 Apr 30 1230 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# http://www.swpc.noaa.gov/wwire.html
#
#             Forecast Discussion
#
Solar Activity

.24 hr Summary...
Solar activity reached moderate levels. Region 3654 (S07W57,
Ekc/beta-gamma-delta) produced an M1.6 flare at 30/0114 UTC. The region
also produced numerous C-class activity including a C8.5/1n at 29/1926
UTC. Region 3654 continued a trend of growth, especially in the
intermediate and trailer spots, and maintained a delta magnetic
configuration in the largest intermediate spot. New Regions 3661
(N23E69, Hsx/alpha) and 3662 (N30E39, Cro/beta) were numbered this
period. The remaining regions were either stable or in decay.

Other activity included an eruption near N13W09 at 29/0909
UTC that displayed a westward flow across GOES-16 SUVI imagery.
SOHO/LASCO imagery showed a CME off the NW limb at 29/1248 UTC that was
modelled as a potential Earth hit early on 03 May. No other
Earth-directed CMEs were detected in available imagery.

.Forecast...
Solar activity is expected to be at low levels over 30 Apr and 01-02 May
with a chance for M-class flare (R1-R2/Minor-Moderate) activity.

Energetic Particles

.24 hr Summary...
The greater than 2 MeV electron flux was at normal to moderate levels
and the greater than 10 MeV proton flux was steady at background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to be at normal to
moderate levels over 30 Apr and 01-02 May. The greater than 10 MeV
proton flux is expected to persist at background levels over 29-30 Apr
and 01 May.

Solar Wind

.24 hr Summary...
The solar wind environment was mildly enhanced due to positive polarity
CH HSS influences. Total field strength reached a peak of 8 nT and the
Bz component was varied between +6/-4 nT. Solar wind speeds remained
steady, averaging about 450 km/s. The phi angle was predominantly
positive throughout the period.

.Forecast...
Enhanced solar wind conditions are likely over 30 Apr and 01-02 May due
to CH HSS influences and possible transient activity.

Geospace

.24 hr Summary...
The geomagnetic field was at quiet levels.

.Forecast...
Geomagnetic field activity is expected to range from quiet to unsettled
levels on 30 Apr, and quiet to active levels on 01-02 May, due to the
anticipated influence of CH HSSs combined with potential transient
activity.